NGC 1910 is an open star cluster located in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. It is situated approximately 160,000 light-years from Earth and is part of a group of clusters known as the LMC Star Clusters. NGC 1910 is notable for its relatively young age, estimated to be around 30 million years. The cluster contains several bright stars and is often studied to understand stellar formation and evolution. It is also associated with the H II region NGC 1910, which is a region of ionized hydrogen gas surrounding the cluster. This makes it an interesting target for astronomers.